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Current astronomical observations are successfully explained by the present cosmological paradigm based on the concordance model ($\Lambda_0$CDM + Inflation). However, such a scenario is composed of a heterogeneous mix of ingredients for…

广义相对论与量子宇宙学 · 物理学 2018-08-29 J. A. S Lima , Douglas Singleton

We present aspects of a model which attempts to unify the creation of cold dark matter, a CP-violating baryon asymmetry, and also a small, residual vacuum energy density, in the early universe. The model contains a primary scalar (inflaton)…

天体物理学 · 物理学 2009-11-13 Saul Barshay , Georg Kreyerhoff

A novel mechanism for explaining the matter-antimatter asymmetry of the universe is considered. We assume that the universe starts from completely symmetric state and then, as it cools down, it undergoes a quantum-phase transition which in…

宇宙学与河外天体物理 · 物理学 2011-05-31 V. R. Shaginyan , G. S. Japaridze , M. Ya. Amusia , A. Z. Msezane , K. G. Popov

Is the Standard Model Charge-Parity (CP) violation ever enough to generate the observed baryon asymmetry? Yes! We introduce a mechanism of baryogenesis (and dark matter production) that can generate the entire observed baryon asymmetry of…

高能物理 - 唯象学 · 物理学 2024-08-26 Gilly Elor , Rachel Houtz , Seyda Ipek , Martha Ulloa

We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath…

高能物理 - 唯象学 · 物理学 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

The origin of matter-antimatter asymmetry is one of the most important outstanding problems at the interface of particle physics and cosmology. Gravitational leptogenesis (baryogenesis) provides a possible mechanism through explicit…

高能物理 - 理论 · 物理学 2015-06-23 J. I. McDonald , Graham M. Shore

The asymmetry between matter and antimatter in the Universe indicates that there was a period in the very early Universe when the CPT symmetry was broken. The conservative interpretation is that the breaking was dynamical, induced by the…

高能物理 - 唯象学 · 物理学 2007-05-23 Robert H. Brandenberger

We propose a new mechanism to simultaneously explain the observed dark matter abundance and the baryon asymmetry of the Universe. The mechanism is based on the Filtered Dark Matter scenario, where dark matter particles acquire a large mass…

高能物理 - 唯象学 · 物理学 2022-08-24 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht , Yotam Soreq

We show how CP violating B meson oscillations in conjunction with baryon number violating decays can generate the cosmological asymmetry between matter and anti-matter, and explore the parameter space of a simple, self-contained model,…

高能物理 - 唯象学 · 物理学 2019-10-09 Ann E. Nelson , Huangyu Xiao

A rapid phase of accelerated expansion in the early universe, known as inflation, dilutes all matter except the vacuum induced quantum fluctuations. These are responsible for seeding the initial perturbations in the baryonic matter, the…

高能物理 - 唯象学 · 物理学 2011-06-28 Anupam Mazumdar

CP violation, which is crucial for producing the baryon asymmetry of the Universe, is enhanced in particle-antiparticle oscillations. We study particle-antiparticle oscillations (of a particle with mass O(100 GeV)) with CP violation in the…

高能物理 - 唯象学 · 物理学 2016-07-01 Seyda Ipek , John March-Russell

In this work we review the theories of origin of matter-antimatter asymmetry in the Universe. The general conditions for achieving baryogenesis and leptogenesis in a CPT conserving field theory have been laid down by Sakharov. In this…

高能物理 - 唯象学 · 物理学 2015-06-17 G. Lambiase , S. Mohanty , A. R. Prasanna

We explore the possibility of baryogenesis without departure from thermal equilibrium. A possible scenario is found, though it contains strong constraints on the size of the $CPT$ violation ($CPTV$) effects and on the role of the $B$…

高能物理 - 理论 · 物理学 2009-11-10 José Manuel Carmona , José Luis Cortés , Ashok Das , Jorge Gamboa , Fernando Méndez

Baryogenesis refers to the theoretical process that occurred in the early history of the universe producing excess of matter over antimatter. Hitherto, fundamental physics which can give rise to such events is unknown. Many theories have…

综合物理 · 物理学 2020-05-13 P. K. Sahoo , Snehasish Bhattacharjee

A popular class of theories attributes the matter-antimatter asymmetry of the Universe to CP-violating decays of super-heavy BSM particles in the Early Universe. Recently, we discovered a new source of leptogenesis in these models, namely…

高能物理 - 唯象学 · 物理学 2017-04-12 J. I. McDonald , G. M. Shore

We introduce an axion-inflation model embedded in the Left-Right symmetric extension of the SM in which $W_R$ is coupled to the axion. This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon…

高能物理 - 唯象学 · 物理学 2021-10-13 Azadeh Maleknejad

We propose that the baryon asymmetry of the Universe may originate from the amplification of quantum fluctuations of a light complex scalar field during inflation. CP-violation is sourced by complex mass terms, which are smaller than the…

天体物理学 · 物理学 2008-12-18 Bjorn Garbrecht , Tomislav Prokopec

The fundamental question of baryogenesis and the problem of matter-antimatter asymmetry motivate this study into the formation and evolution of antimatter objects in the early Universe. Hypothesize is the existence of isolated antimatter…

高能天体物理现象 · 物理学 2026-02-04 Sattvik Yadav

We propose a new mechanism to generate a lepton asymmetry based on the vacuum CP-violating phase transition (CPPT). This approach differs from classical thermal leptogenesis as a specific seesaw model, and its UV completion, need not be…

高能物理 - 唯象学 · 物理学 2018-03-14 Silvia Pascoli , Jessica Turner , Ye-Ling Zhou

We review observational evidence for a matter-antimatter asymmetry in the early universe, which leads to the remnant matter density we observe today. We also discuss observational bounds on the presence of antimatter in the present day…

高能物理 - 唯象学 · 物理学 2012-11-06 Laurent Canetti , Marco Drewes , Mikhail Shaposhnikov
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